SDO HMI 2014-10-29 00:00:29 UT
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| group | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 14.74 | 40.92 | 7.61 | 21.29 | -3.18 | 160.04 | -15.33 | 117.60 | 0.2978 | 710.4 | 458.5 | |
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| spot | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 0.00 | 1.13 | 0.00 | 0.57 | -2.18 | 166.44 | -8.93 | 127.51 | 0.1964 | 822.0 | 562.6 | |
| 0.00 | 1.04 | 0.00 | 0.53 | -2.19 | 166.23 | -9.14 | 126.87 | 0.1993 | 791.0 | 651.2 | |
| 14.74 | 22.90 | 7.61 | 11.82 | -3.47 | 161.13 | -14.24 | 119.64 | 0.2838 | 1230.1 | 688.5 | |
| 0.00 | 1.99 | 0.00 | 1.03 | -1.56 | 160.48 | -14.89 | 112.51 | 0.2793 | 790.0 | 535.7 | |
| 0.00 | 0.95 | 0.00 | 0.49 | -1.27 | 160.26 | -15.11 | 111.24 | 0.2808 | 890.0 | 781.2 | |
| 0.00 | 3.90 | 0.00 | 2.02 | -1.81 | 159.86 | -15.51 | 112.48 | 0.2906 | 445.0 | 489.0 | |
| 0.00 | 1.21 | 0.00 | 0.63 | -4.67 | 159.81 | -15.56 | 120.89 | 0.3130 | 582.0 | 482.8 | |
| 0.00 | 1.39 | 0.00 | 0.72 | -1.54 | 159.80 | -15.57 | 111.54 | 0.2898 | 783.0 | 552.8 | |
| 0.00 | 1.47 | 0.00 | 0.77 | -4.53 | 159.50 | -15.87 | 120.00 | 0.3161 | 924.0 | 749.5 | |
| 0.00 | 0.78 | 0.00 | 0.41 | -2.78 | 159.47 | -15.90 | 114.94 | 0.3031 | 694.0 | 607.6 | |
| 0.00 | 0.95 | 0.00 | 0.50 | -4.59 | 159.25 | -16.12 | 119.79 | 0.3203 | 926.0 | 788.5 | |
| 0.00 | 1.13 | 0.00 | 0.60 | -3.12 | 155.52 | -19.85 | 111.17 | 0.3652 | -760.0 | -575.2 | |
| 0.00 | 0.95 | 0.00 | 0.55 | -4.70 | 146.95 | -28.42 | 107.93 | 0.5006 | -904.0 | -781.6 | |
| 0.00 | 1.13 | 0.00 | 0.65 | -4.67 | 146.71 | -28.66 | 107.75 | 0.5039 | -703.0 | -571.2 | |
| Proj. U | - Projected umbra area in millionths of solar disc, negative values indicate | |
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that the umbra consists of fragmented regions which cannot be separated without losing umbral area. In this way several spots (intensity minima in the umbra) have a common umbra, e.g. -2 means that the given spot shares an umbra with spot No.2, and the common U value is indicated at spot No.2. |
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| Proj. WS | - Projected whole spot area in millionths of solar disc, negative values indicate | |
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that several umbras have a common penumbra, e.g. -7 means that the given umbra shares a penumbra with umbra No.7, and the WS value is indicated at No.7. |
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| Corr. U | - Corrected umbra area in millionths of solar hemisphere, for negative values see above | |
| Corr. WS | - Corrected whole spot area in millionths of solar hemisphere, for negative values see above | |
| B | - Heliographic latitude B; positive: North, negative: South | |
| L | - Heliographic longitude L | |
| LCM | - Longitudinal distance from the Sun's central meridian | |
| Pos. angle | - Position angle | |
| r | - Distance from the centre of Sun's disc in terms of Sun's radius | |
| MU | - Mean magnetic field within the umbra contour averaged the pixel values with sign. | |
| MP | - Mean magnetic field within the penumbra contour averaged the pixel values with sign. | |